English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse
  1. View item / 
  2. Item Summary

Item

ITEM ACTIONSEXPORT
Add to Basket
  Local TagsRelease HistoryDetailsSummary

Released
Conference Paper

Periodicity Analysis of Mrk 501 and Mrk 421 in Gamma Rays

MPS-Authors
/persons/resource/persons230577

Arras,  P.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

/persons/resource/persons16142

Ensslin,  T.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

/persons/resource/persons269334

Kostić,  A.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

External Resource
No external resources are shared
Fulltext (restricted access)
There are currently no full texts shared for your IP range.
Fulltext (public)
There are no public fulltexts stored in PuRe
Supplementary Material (public)
There is no public supplementary material available
Citation

Iotov, R., Arbet-Engels, A., Arras, P., Baack, D., Balbo, M., Biland, A., et al. (2022). Periodicity Analysis of Mrk 501 and Mrk 421 in Gamma Rays. Proceedings of Science, 395: 879. doi:10.22323/1.395.0879.


Cite as: https://hdl.handle.net/21.11116/0000-000E-0EE8-E
Abstract
Blazars, a subclass of active galactic nuclei (AGNs), are highly variable objects. Quasiperiodic oscillations (QPOs), which might originate from a binary black hole located at the AGN core,have been found in some blazar light curves. For the blazars Mrk 421 and Mrk 501, we test the possible QPO behavior using a variety of methods (generalized Lomb-Scargle periodogram,continuous-time autoregressive moving average models, wavelet scalograms, and A−T plane), studying systematic effects in detail. We use gamma-ray light curves from FACT, a ground-based imaging air